scholarly journals Performance of GPS slant total electron content and IRI-Plas-STEC for days with ionospheric disturbance

2016 ◽  
Vol 7 (1) ◽  
pp. 1-10 ◽  
Author(s):  
Feza Arikan ◽  
Seymur Shukurov ◽  
Hakan Tuna ◽  
Orhan Arikan ◽  
T.L. Gulyaeva
2017 ◽  
Vol 35 (3) ◽  
pp. 345-351 ◽  
Author(s):  
Ayman Mahrous

Abstract. This paper presents observational evidence of frequent ionospheric perturbations caused by the magnetar flare of the source SGR J1550–5418, which took place on 22 January 2009. These ionospheric perturbations are observed in the relative change of the total electron content (ΔTEC/Δt) measurements from the coherent ionospheric Doppler radar (CIDR). The CIDR system makes high-precision measurements of the total electron content (TEC) change along ray-paths from ground receivers to low Earth-orbiting (LEO) beacon spacecraft. These measurements can be integrated along the orbital track of the beacon satellite to construct the relative spatial, not temporal, TEC profiles that are useful for determining the large-scale plasma distribution. The observed spatial TEC changes reveal many interesting features of the magnetar signatures in the ionosphere. The onset phase of the magnetar flare was during the CIDR's nighttime satellite passage. The nighttime small-scale perturbations detected by CIDR, with ΔTEC/Δt  ≥  0.05 TECU s−1, over the eastern Mediterranean on 22 January 2009 were synchronized with the onset phase of the magnetar flare and consistent with the emission of hundreds of bursts detected from the source. The maximum daytime large-scale perturbation measured by CIDR over northern Africa and the eastern Mediterranean was detected after ∼ 6 h from the main phase of the magnetar flare, with ΔTEC/Δt  ≤  0.10 TECU s−1. These ionospheric perturbations resembled an unusual poleward traveling ionospheric disturbance (TID) caused by the extraterrestrial source. The TID's estimated virtual velocity is 385.8 m s−1, with ΔTEC/Δt  ≤  0.10 TECU s−1.


Space Weather ◽  
2014 ◽  
Vol 12 (1) ◽  
pp. 64-75 ◽  
Author(s):  
Hakan Tuna ◽  
Orhan Arikan ◽  
Feza Arikan ◽  
Tamara L. Gulyaeva ◽  
Umut Sezen

2006 ◽  
Vol 81 (2) ◽  
pp. 111-120 ◽  
Author(s):  
L. Ciraolo ◽  
F. Azpilicueta ◽  
C. Brunini ◽  
A. Meza ◽  
S. M. Radicella

2009 ◽  
Vol 49 (4-5) ◽  
Author(s):  
M. A. Cabrera ◽  
R. G. Ezquer ◽  
P. Spalla

GPS Solutions ◽  
2018 ◽  
Vol 22 (3) ◽  
Author(s):  
Wenfeng Nie ◽  
Tianhe Xu ◽  
Adria Rovira-Garcia ◽  
José Miguel Juan Zornoza ◽  
Jaume Sanz Subirana ◽  
...  

2019 ◽  
Vol 11 (12) ◽  
pp. 1497 ◽  
Author(s):  
Yan Xiang ◽  
Yang Gao

Mapping function (MF) converts the line-of-sight slant total electron content (STEC) into the vertical total electron content (VTEC), and vice versa. In an MF, an essential parameter is the ionospheric effective height. However, the inhomogeneous ionosphere makes this height vary spatially and temporally, meaning it is not a global constant. In the paper, we review several mapping functions and propose a mapping function that utilizes the ionospheric varying height (IVH). We investigate impacts of the IVH on mapping errors and on the ionospheric modeling, as well as on the satellite and receiver differential code biases (DCBs). Our analysis results indicate that the mapping errors using IVH are smaller than those from the fixed height of 450 km. The integral height achieves smaller mapping errors than using a fixed height of 450 km, an improvement of about 8% when compared with the fixed height of 450 km. And 35% smaller mapping errors were found using HmF2 at the lower latitude. Also, the effects of IVH on the satellite DCBs are about 0.1 ns, and larger impacts on the receiver DCBs at 1.0 ns.


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